THE EXTREME SPIN OF THE BLACK HOLE IN CYGNUS X-1

Record Type
Journal Articles
Full Title
THE EXTREME SPIN OF THE BLACK HOLE IN CYGNUS X-1
Author(s)
Gou L, McClintock J, Reid M, Orosz J, Steiner J, Narayan R, Xiang J, Remillard R, Arnaud K, Davis S
Publication Title
ASTROPHYSICAL JOURNAL
Publication Title (abbreviated)
ASTROPHYS J
Publication Date
2011 Dec 1
DOI
10.1088/0004-637X/742/2/85
ISSN
0004-637X
Volume
742
Issue
2
Page Count
17
Article Number
85
Keyword(s)
Astronomy & Astrophysics, accretion, accretion disks, black hole physics, stars: individual (Cygnus X-1), X-rays: binaries, X-RAY BINARIES, CONTINUUM-FITTING METHOD, ACCRETION DISK MODELS, DWARF NOVA OUTBURSTS, EMISSION-LINES, INNER-DISK, SOFT STATE, LMC X-1, MASS, REFLECTION
Citation
Gou L, McClintock J, Reid M, Orosz J, Steiner J, Narayan R, Xiang J, Remillard R, Arnaud K, Davis S. THE EXTREME SPIN OF THE BLACK HOLE IN CYGNUS X-1. ASTROPHYS J. 2011;742 (2):17.
Conditions of Use
  • Author can archive pre-print (i.e., pre-refereeing)
  • Author can archive post-print (i.e., final draft post-refereeing)
  • On any website, arXiv, scientific social networks (except Research Gate) or non-commercial open access repository.
  • Publisher's version/PDF may be used on any website or authors' institutional repository
  • Publisher copyright and source must be acknowledged
  • Must link to publisher version
  • Publisher's version/PDF may be used
  • Authors depositing in arXiv must they choose the first licence statement offered by arXiv when uploading their article – a "non-exclusive licence to distribute"
  • Publisher last contacted on 10/02/2016

More usage information may be available at SHERPA/RoMEO